Statistical characteristics of a stochastic background of gravitational waves from neutron star formation

被引:6
|
作者
Coward, D [1 ]
Burman, R [1 ]
Blair, D [1 ]
机构
[1] Univ Western Australia, Dept Phys, Nedlands, WA 6009, Australia
关键词
D O I
10.1088/0264-9381/19/7/310
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
By using a recent model for the evolving star formation rate, we investigate the statistical distribution of gravitational wave amplitudes due to supernovae that result in neutron star formation in the Einstein-de Sitter cosmiology. To account for the uncertainty in gravitational wave emission for this source type, we use a random mixture of three simulated waveform types computed by Zwerger and Muller. We investigate statistical parameters of the resulting gravitational wave amplitude distribution in our frame.
引用
收藏
页码:1303 / 1307
页数:5
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